4.8 Article

Observation of an Excited Ω- Baryon

期刊

PHYSICAL REVIEW LETTERS
卷 121, 期 5, 页码 -

出版社

AMER PHYSICAL SOC
DOI: 10.1103/PhysRevLett.121.052003

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资金

  1. Ministry of Education, Culture, Sports, Science, and Technology (MEXT) of Japan
  2. Japan Society for the Promotion of Science (JSPS)
  3. Tau-Lepton Physics Research Center of Nagoya University
  4. Australian Research Council
  5. Austrian Science Fund [P 26794-N20]
  6. National Natural Science Foundation of China [11435013, 11475187, 11521505, 11575017, 11675166, 11705209]
  7. Key Research Program of Frontier Sciences, Chinese Academy of Sciences (CAS) [QYZDJ-SSW-SLH011]
  8. CAS Center for Excellence in Particle Physics (CCEPP)
  9. Fudan University [JIH5913023, IDH5913011/003, JIH5913024, IDH5913011/002]
  10. Ministry of Education, Youth and Sports of the Czech Republic [LTT17020]
  11. Carl Zeiss Foundation
  12. Deutsche Forschungsgemeinschaft
  13. Excellence Cluster Universe
  14. VolkswagenStiftung
  15. Department of Science and Technology of India
  16. Instituto Nazionale di Fisica Nucleare of Italy
  17. National Research Foundation (NRF) of Korea [2014R1A2A2A01005286, 2015R1A2A2A01003280, 2015H1A2A1033649, 2016R1D1A1B01010135, 2016K1A3A7A09005 603, 2016R1D1A1B02012900]
  18. Radiation Science Research Institute, Foreign Large-size Research Facility Application Supporting project
  19. Global Science Experimental Data Hub Center of the Korea Institute of Science and Technology Information
  20. Polish Ministry of Science and Higher Education
  21. National Science Center
  22. Russian Federation Government [14.W03.31.0026]
  23. Slovenian Research Agency
  24. Ikerbasque, Basque Foundation for Science, Basque Government [IT956-16]
  25. Ministry of Economy and Competitiveness (MINECO) (Juan de la Cierva), Spain
  26. Swiss National Science Foundation
  27. Ministry of Education
  28. Ministry of Science and Technology of Taiwan
  29. U.S. Department of Energy
  30. National Science Foundation

向作者/读者索取更多资源

Using data recorded with the Belle detector, we observe a new excited hyperon, an Omega*(-) candidate decaying into Xi K-0(-) and Xi K--(S)0 with a mass of 2012.4 +/- 0.7(stat) +/- 0.6(syst) McV/c(2) and a width of Gamma = 6.4(-2.0)(+2.5)(stat) +/- 1.6(syst) MeV. The Omega*(-) is seen primary in gamma(1S), gamma(2S), and gamma(3S) decays.

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